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Evolution of gravitational waves in Randall-Sundrum cosmology

Richard Easther·David Langlois·Roy Maartens·David Wands
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Abstract

We investigate the evolution of gravitational wave perturbations about a brane cosmology embedded in a five-dimensional anti-de Sitter bulk. During slow-roll inflation in a Randall-Sundrum brane-world, the zero mode of the 5-dimensional graviton is generated, while the massive modes remain in their vacuum state. When the zero mode re-enters the Hubble radius during radiation domination, massive modes are generated. We show that modes decouple in the low-energy/near-brane limit and develop perturbative techniques to calculate the mode-mixing at finite energy.

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Richard Easther, David Langlois, Roy Maartens, David Wands. 2003-08-12. Evolution of gravitational waves in Randall-Sundrum cosmology. https://doi.org/10.1088/1475-7516%2F2003%2F10%2F014

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